Investigation of the Venus atmosphere and surface by the method of radiosounding using Venera-9 and 10 satellites

Using the Venera-9 and 10 satellites radio occultation measurements of the atmosphere and bistatic radar measurements of the surface of the planet Venus were realized from October 1975 to March 1976. The altitude dependence of the molecular number density, pressure and temperature on the night and day sides were derived.An analysis is made of the stratified structure and turbulence in the atmosphere of Venus. The results of pressure measurements on the surface by the method of bistatic radar are presented. The diagrams and the tables of the parameters of the atmosphere are given.     

大气环境电子束材料表面强化机理数值模拟

建立了大气环境电子束材料表面强化过程的多阶段数值模型,用于对电子束与材料表面层的相互作用过程和结构与相变过程进行研究。通过应用这一模型,使得对材料表面强化中电子束传输、温度演化和相变动力学等多参数研究成为可能,由此建立了电子束输入参数与结构相变结果之间的关系。     

Speeding up the Development of Space Industry to Meet the New Challenge

This paper discusses the urgency to further develop China's space technological industry;analyzes the gaps between China and other advanced countries in space industry,including technological level,development scale,application scope and investment;describes the current severe situation that the China's space industry is faced with and proposes the overall objective,guiding principles and major tasks of China's space technological sector in the Ninth-Five Year Plan and the coming decade.Finally,it proposes some policies and effective measures to speed up the development of China's space industry to meet the challenge in the 21st century.     

Transient flashes of electromagnetic radiation in the upper atmosphere

Experimental data related to electric discharges in the upper atmosphere are considered. These discharges occupy enormous volumes of the atmosphere (up to 1000 km³) and are accompanied by optical radiation (in the UV, optical, and IR ranges), and also by gamma-ray radiation. Possible physical processes responsible for the evolution of such discharges are also considered.     

Determination of the width of a corridor of re-entry into the atmosphere for the problem of launching a spacecraft into a circumplanetary orbit after braking in the atmosphere

A method of calculating the optimal trajectories of a spacecraft re-entry into the atmosphere is considered under the condition of minimization of a re-orbit burn at the apocenter of the segment of escape from the atmosphere and taking into account a constraint on the maximum overload.     

Drying as one of the extreme factors for the microflora of the atmosphere

An investigation of the effects of drying and drying-rewetting cycles under vacuum conditions of 10(-2) torr at -30 degrees C on conidia of the atmospheric strain Penicillium chrysogenum from 48-77 km heights, collected by meteorological rockets found that survival and restoration of the initial physiological properties were possible through some very efficient protective cellular mechanisms. Such adaptive possibilities explain the widespread diffusion of microbial cells throughout the biosphere of our planet.     

Ascending flows in the solar atmosphere and formation of the solar wind

Some morphological features of solar magnetic fields in the chromosphere and corona are considered based on studying various observational data. These data are compared to the results of observation of the solar wind and interplanetary magnetic field, as well as to the data on fluxes of solar cosmic rays. New specific features are found in the solar wind structure, and new additional indications of sources of the solar wind are obtained. The properties of the active regions and coronal holes are considered. A model of the ascending stream-like plasma flow is suggested. It flows around the discrete arched magnetic field tubes in the solar atmosphere and stretches them out into interplanetary space.     

Statistical analysis of attitude motion of a light capsule entering the atmosphere

The laws of distribution of the space angle of attack are analyzed for a light descent capsule on the atmosphere’s conventional boundary and on the segment of motion in dense layers of the atmosphere until the moment of reaching the maximum velocity head. It is assumed that upon detachment from a base spacecraft the angular velocity components of the descent capsule represent independent random quantities distributed according to the normal law. The shape of the descent capsule is close to a body of revolution whose instantaneous aerodynamic characteristic has a sufficiently simple form (one stable and one unstable positions of static equilibrium). It is demonstrated that there is a possibility to approximate the distribution densities by well-known laws and by approximate functions constructed on the basis of simplified models. Evolution of the distribution laws at increasing mass-inertia asymmetry of the descent capsule is studied.     

变结构控制在导弹总线网络控制中的应用研究

随着导弹数字控制技术和网络通信技术的发展,数据总线传输方案越来越受到重视.以数据总线为核心的导弹总线网络控制系统能够有效克服传统通信网络的弊端,改善系统性能,然而由于信息传输分时复用通信网络,系统延时是不可避免的.本文利用接收缓冲区,将时变延时转变为固定延时,并在此基础上,对导弹总线网络控制系统提出滑模预估控制器设计方法.仿真结果表明,这种设计方法是有效的.     

Features of rotational motion of a spacecraft descending in the Martian atmosphere

Angular motion at atmospheric entry is studied in the paper for a spacecraft with a bi-harmonic moment characteristic. Special attention is given to the case when the spacecraft possesses two stable balanced positions, and, hence, it can oscillate in dense atmospheric layers in the ranges of small or large angles of attack. The averaged equations of spacecraft motion are derived, which allow one to increase the speed of calculations by several orders of magnitude. A real example is presented, which concerns a spacecraft specially designed for descending in the Martian atmosphere.     

Development of a complex prognostic model of the upper atmosphere and ionosphere

We consider possible stages of constructing complex models of the circumterrestrial plasma including both neutral and charged components in their interaction. At the initial stage it is suggested to use as a basis the empirical models of the upper atmosphere and ionosphere. These models have concentrated fundamental data about the near-Earth space (NES) accumulated for several decades of space exploration. The final goal is to construct a prognostic model which would allow one to calculate both long-periodic variations of the NES structure (they can occur over several decades of years and more) and short-period disturbances with a characteristic time of about a day. In order to predict the results of anthropogenic effects it is proposed to construct imitation mathematical models that should allow one to calculate NES variations which can proceed at various model scenarios of anthropogenic actions.     

从句法的角度看汉语动语语法化的机制

论文通过讨论汉语动词语法化的进程,说明动词句法演变的机制以及导致演变的诱因。     

Problems related to non-linear variations of surface tension

Generally, the tension at a liquid/gas interface is decreasing with temperature. For aqueous solution of alcohol, alkylammonium chloride in water, some binary metallic alloys and nematic liquid crystals the surface tension presents an extremum as a function of temperature. The influence of this property on the hydrodynamic stability and on the surface tension induced flows is studied as well theoretically as experimentally.     

长征系列运载火箭航天发射总次数突破两位数

长征系列火箭为中国航天运载火箭的统称。文章讨论了该系列火箭的组成和航天发射情况。     

一种非数据辅助前向结构载波频偏估计的算法

文章给出了一种适用于MPSK解调的非数据辅助(NDA)载波频偏估计算法,该算法采用前向开环载波同步方式,利用相邻样本之间的相关信息提取载波频偏,具有同步速度快、载波频偏估计范围大、计算量小、可全数字化的优点,适用于高速突发数字通信系统.通过计算机仿真.给出了该算法在估计范围、估计精度方面的性能.     

One method of controlling the motion of an aerospace vehicle during its long flight in the atmosphere

Based on the methods of the theory of optimum control of dynamic systems, as well as the methods of inverse problems of dynamics and the energy principle, a combined method is developed for control of the motion of a flying vehicle of the Aerospace plane type during the long flight in the atmosphere. The disturbed motion is considered under the conditions when there are constraints on the values of control actions and on functions of phase coordinates.     

Structure of the Disturbed Magnetosphere

The quasitrapping region (QTR) at the night side of a disturbed magnetosphere in the majority of models is either absent completely or merges with the plasma sheet of the magnetosphere tail. At the same time these two regions are different both in the topology of the magnetic field and in the character of motion of charged particles. Moreover, it is the region of quasitrapping that is conjugate to the zone of auroral active forms; i.e., it can be called the auroral magnetosphere. Models of the magnetosphere in which the tail structures of the magnetic field are directly adjacent to the boundary of stable trapping (in particular, the isotropic boundary model) are based on erroneous assumptions. Our understanding of the processes of magnetosphere substorms and magnetic storms depends on a correct understanding of the magnetosphere structure.